that \(M\)  is the mass of black hole, \(g\)  is the magnetic charge of black hole and \(a\)  and \(\omega \)  are the normalization factor and the state parameter of the quintessence matter, respectively. In the case of \(a = 0\) , the above metric reduces to the Hayward black hole obtained by Hayward [1]}, and for \(g=0\)  represents the Schwarzschild black hole surrounded by quintessence matter that was initially obtained by Kiselve in [2]}. Also, for \(a=g=0\)  behaves like the Schwarzschild black hole that has only one event horizon. We also note by choosing different values of \(\omega \) , the different black hole solutions can be obtained. For instance, when \(\omega =-\frac{1}{3}\)  the solution (REF ) corresponds to the Hayward black hole [1]} and for \(\omega =-1\)  and \(a=\frac{\Lambda }{3}\)  reduces to the Hayward de Sitter solution. Moreover, in the case of \(\omega =\frac{1}{3}\)  and \(a=-Q^2\)  corresponds to the charged Hayward black hole [4]}.
